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Titlebook: Atomic and Nuclear Physics; An Introduction T. A. Littlefield,N. Thorley Book 1979Latest edition Springer Science+Business Media New York 1

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發(fā)表于 2025-3-21 16:36:57 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
期刊全稱(chēng)Atomic and Nuclear Physics
期刊簡(jiǎn)稱(chēng)An Introduction
影響因子2023T. A. Littlefield,N. Thorley
視頻videohttp://file.papertrans.cn/165/164796/164796.mp4
圖書(shū)封面Titlebook: Atomic and Nuclear Physics; An Introduction T. A. Littlefield,N. Thorley Book 1979Latest edition Springer Science+Business Media New York 1
影響因子After the death of Dr. Littlefield it was decided that I should undertake the revision ofthe whole of Atomic and Nuclear Physics: an Introduction for the third edition, and it was soon apparent that major changes were necessary. I am confident that these changes would have had Dr. Littlefield‘s approval. The prime consideration for the present edition has been to modernize at a minimum cost. As much as possible of the second edition has therefore been retained, but where changes have been made they have been fairly drastic. Thus the chapters on fine structure, wave mechanics, the vector model of the atom, Pauli‘s principle and the Zeeman effect have been completely restructured. The chapters on nuclear models, cosmic rays, fusion systems and fundamental particles have been brought up to date while a new chapter on charm and the latest ideas on quarks has been included. It is hoped that the presentation of the last named will give readers a feeling that physics research can be full of adventure and surprises.
Pindex Book 1979Latest edition
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The Electromagnetic Spectrum, it is converted into heat, a form of energy. Energy must therefore have arrived from the sun across this immense distance. In fact almost all the energy known to man has been derived from the sun either now or in past ages. Thus the sun’s energy, which millions of years ago was responsible for the
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Spectra,rning the distribution of lines in a spectrum was discovered by Balmer and Rydberg. The interpretation of this law in terms of atomic structure began with the work of Bohr in 1913. It revealed that a study of spectra could provide a wealth of information about atomic structure. Hydrogen, being the s
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Fine Structure and Electron Spin,own that the first member of the principal series is the sodium yellow line, which, with quite moderate resolving power, is seen to consist of two lines separated by about 0?6 nm. These are the well-known D-lines at 589·0 and 589·6 nm. All lines in the principal, sharp and diffuse series are doublet
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Waves and Particles,ctricity, in the Compton effect and in the continuous spectrum of X-rays. This is supported and extended by the wealth of experimental data arising from the study of optical and X-ray line spectra. However, the phenomena of interference, diffraction and polarization still require a wave theory for t
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